| NGC 720 | |
|---|---|
 NGC 720 byChandra X-ray Observatory (left) andDSS (right) | |
| Observation data (J2000epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 53m 00.5s[1] |
| Declination | −13° 44′ 19″[1] |
| Redshift | 0.005821 +/- 0.000022[1] |
| Heliocentric radial velocity | 1,745 ± 7km/s[1] |
| Distance | 80 ± 20Mly (24.4 ± 6.3Mpc)[1] |
| Apparent magnitude (V) | 10.2 |
| Characteristics | |
| Type | E5[1] |
| Apparent size (V) | 4.7′ × 2.4′[1] |
| Notable features | StrongX-rays source |
| Other designations | |
| MCG -02-05-068,PGC 6983[1] | |
NGC 720 is anelliptical galaxy located in the constellationCetus. It is located at a distance of circa 80 millionlight years from Earth, which, given its apparent dimensions, means that NGC 720 is about 110,000 light years across.[1] It was discovered byWilliam Herschel on October 3, 1785.[2] The galaxy is included in theHerschel 400 Catalogue. It lies about three and a half degrees south and slightly east fromzeta Ceti.[3]
NGC 720 is an elliptical galaxy with elongated shape in the northwest to southeast axis as seen from Earth.[3] Observations by theHubble Space Telescope of the core of NGC 720 did not reveal the presence of dust, disk, orinner spiral.[4] As observed in X-rays by theChandra X-ray Observatory in 2000, the galaxy features a slightly flattened, or ellipsoidal triaxial halo of hot gas that has an orientation different from that of the optical image of the galaxy. The observations by Chandra X-ray Observatory fit predictions of acold dark matter model.[5][6] Although the data also fit the expectations frommodified Newtonian dynamics (MOND).[7] The galaxy lacks emission inradio waves, meaning it does not host anactive galactic nucleus. The total mass of the galaxy with its dark matter halo is estimated to be(3.1±0.4)×1012M☉, with the total gas mass exceeding the stellar one. The observations of hot gas fit models that are nearlyhydrostatic.[8] 42 X-ray point sources were detected in the galaxy, including a possible central source. Twelve of them are located within 2 arcsec of globular cluster candidates. NGC 720 features nineultraluminous X-ray sources, the most found in anearly type galaxy as of 2003.[9]
Observations made in 1996 suggested the galaxy had 660 ±190globular clusters in the central 30kpc, a number considered small for such a galaxy. The allocation of the clusters resembled the ellipticity, position angle and surface brightness of the galaxy.[10] However, in 2012 it was observed that the blue globular clusters subpopulation had a similar slope with the X-ray surface brightness profile.[11] Further observations by the SLUGGS Survey (2016), with wider field data, raised the number of globular clusters in the galaxy to 1489 ± 96 and their distribution was less elliptical than the surface profile of the galaxy. The clusters have bimodal distribution as far as color is concerned, with the clusters characterised as red or blue, with the blue clusters having a stronger connection with the galactic halo.[12]
Optical long slitspectrography of the galaxy showed a strong age gradient along the semimajor axis of NGC 720, which has been explained on the grounds of two distinct population components. At the centre of the galaxy lie stars whose age is estimated to be 13 billion years (Gyrs) old up to 0.73 kpc, where stars with solarmetallicity age (5 Gyrs) dominate. These older stars form a small bulge-like spheroid. At distances over 1 kpc dominate stars with age at 2,5 Gyrs. Based on the Mg2 gradient and its mass, it is proposed that NGC 720 underwent an unequal massgalaxy merger about 4 Gyrs ago.[13]
NGC 720 is the foremost galaxy in a smallgalaxy group, the NGC 720 group, which also includes the galaxyArp 4.[14] NGC 720 lies at the centre of the group and the rest of the galaxies of the group aredwarf galaxies, which are at least 2 mag fainter than NGC 720. There is extended intragroup X-ray emission. The high fraction of early-type galaxies suggest that NGC 720 may be a fossil group, despite its low mass.[15] Further away lie the edge-on spiral galaxyNGC 681,NGC 701, andNGC 755.[14]
